Microcontinent formation around Australia

Microcontinents are common in the accreted continental geological record, but relatively rare in modern settings. Many of today's microcontinents are found in the Tasman Sea and Indian Ocean. These include the East Tasman Rise, the Gilbert Seamount Complex, the Seychelles, Elan Bank (Kerguelen...

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Main Authors: Gaina, C., Müller, R. D., Brown, B., Ishihara, T.
Other Authors: Hillis, R. R., Muller, R. D.
Format: Book Part
Language:unknown
Published: Geological Society of America 2003
Subjects:
Online Access:https://eprints.qut.edu.au/234263/
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spelling ftqueensland:oai:eprints.qut.edu.au:234263 2024-02-04T09:55:42+01:00 Microcontinent formation around Australia Gaina, C. Müller, R. D. Brown, B. Ishihara, T. Hillis, R. R. Muller, R. D. 2003 https://eprints.qut.edu.au/234263/ unknown Geological Society of America doi:10.1130/0-8137-2372-8.405 Gaina, C., Müller, R. D., Brown, B., & Ishihara, T. (2003) Microcontinent formation around Australia. In Hillis, R. R. & Muller, R. D. (Eds.) Evolution and Dynamics of the Australian Plate. Geological Society of America, United States of America, pp. 405-416. https://eprints.qut.edu.au/234263/ 2003 Geological Society of America, Inc. This work is covered by copyright. Unless the document is being made available under a Creative Commons Licence, you must assume that re-use is limited to personal use and that permission from the copyright owner must be obtained for all other uses. If the document is available under a Creative Commons License (or other specified license) then refer to the Licence for details of permitted re-use. It is a condition of access that users recognise and abide by the legal requirements associated with these rights. If you believe that this work infringes copyright please provide details by email to qut.copyright@qut.edu.au Evolution and Dynamics of the Australian Plate Hot spots Microcontinent Riffing Sea-floor spreading Chapter in Book, Report or Conference volume 2003 ftqueensland https://doi.org/10.1130/0-8137-2372-8.405 2024-01-09T00:09:21Z Microcontinents are common in the accreted continental geological record, but relatively rare in modern settings. Many of today's microcontinents are found in the Tasman Sea and Indian Ocean. These include the East Tasman Rise, the Gilbert Seamount Complex, the Seychelles, Elan Bank (Kerguelen Plateau), and possibly fragments of the Lord Howe Rise and Norfolk Ridge, and the Wallaby Plateau. We review their history of formation, and propose that the mechanisms that led to their isolation were mostly plume-related. Tasman Sea continental fragments formed by ridge jumps onto adjacent continental margins after sea-floor spreading in the southern Tasman Sea commenced. The East Tasman Plateau was separated from the Lord Howe Rise at about chron 34 (83 Ma) and the Gilbert Seamount Complex rifted off the South Tasman Rise at roughly 77 Ma, by ridge jumps in opposing directions. Evidence for thermal anomalies under the central Lord Howe Rise, Ross Sea and possible eastern Australian margin explain ridge jumps that led to the isolation of the East Tasman Plateau, Gilbert Seamount and possibly the northern Lord Howe Rise and Dampier Ridge. In the central Indian Ocean, spectacular exposures of granite make the Seychelles a type example of a microcontinent. As in the Tasman Sea, ridge-plume interactions have been responsible for separating a thinned continental sliver from a large continent (India). Elan Bank, as part of the Kerguelen Plateau, represents another example of a continental fragment in the Indian Ocean. Newly identified M-sequence anomalies in the Enderby Basin, off Antarctica, suggest that this microcontinent was detached from India no earlier than 124 Ma when a northward ridge jump towards the Kerguelen plume may have isolated Elan Bank. This Interpretation implies that a mantle thermal anomaly due to the incipient Kerguelen plume pre-dated the Rajmahal Traps, emplaced at about 118 Ma, by ∼6 million years. An early Kerguelen hot-spot position north of Elan Bank, with subsequent southward migration, is also ... Book Part Antarc* Antarctica Ross Sea Queensland University of Technology: QUT ePrints Ross Sea Kerguelen Indian South Tasman Rise ENVELOPE(148.000,148.000,-47.500,-47.500) Elan Bank ENVELOPE(67.000,67.000,-56.750,-56.750) Gilbert Seamount ENVELOPE(-150.083,-150.083,52.833,52.833)
institution Open Polar
collection Queensland University of Technology: QUT ePrints
op_collection_id ftqueensland
language unknown
topic Hot spots
Microcontinent
Riffing
Sea-floor spreading
spellingShingle Hot spots
Microcontinent
Riffing
Sea-floor spreading
Gaina, C.
Müller, R. D.
Brown, B.
Ishihara, T.
Microcontinent formation around Australia
topic_facet Hot spots
Microcontinent
Riffing
Sea-floor spreading
description Microcontinents are common in the accreted continental geological record, but relatively rare in modern settings. Many of today's microcontinents are found in the Tasman Sea and Indian Ocean. These include the East Tasman Rise, the Gilbert Seamount Complex, the Seychelles, Elan Bank (Kerguelen Plateau), and possibly fragments of the Lord Howe Rise and Norfolk Ridge, and the Wallaby Plateau. We review their history of formation, and propose that the mechanisms that led to their isolation were mostly plume-related. Tasman Sea continental fragments formed by ridge jumps onto adjacent continental margins after sea-floor spreading in the southern Tasman Sea commenced. The East Tasman Plateau was separated from the Lord Howe Rise at about chron 34 (83 Ma) and the Gilbert Seamount Complex rifted off the South Tasman Rise at roughly 77 Ma, by ridge jumps in opposing directions. Evidence for thermal anomalies under the central Lord Howe Rise, Ross Sea and possible eastern Australian margin explain ridge jumps that led to the isolation of the East Tasman Plateau, Gilbert Seamount and possibly the northern Lord Howe Rise and Dampier Ridge. In the central Indian Ocean, spectacular exposures of granite make the Seychelles a type example of a microcontinent. As in the Tasman Sea, ridge-plume interactions have been responsible for separating a thinned continental sliver from a large continent (India). Elan Bank, as part of the Kerguelen Plateau, represents another example of a continental fragment in the Indian Ocean. Newly identified M-sequence anomalies in the Enderby Basin, off Antarctica, suggest that this microcontinent was detached from India no earlier than 124 Ma when a northward ridge jump towards the Kerguelen plume may have isolated Elan Bank. This Interpretation implies that a mantle thermal anomaly due to the incipient Kerguelen plume pre-dated the Rajmahal Traps, emplaced at about 118 Ma, by ∼6 million years. An early Kerguelen hot-spot position north of Elan Bank, with subsequent southward migration, is also ...
author2 Hillis, R. R.
Muller, R. D.
format Book Part
author Gaina, C.
Müller, R. D.
Brown, B.
Ishihara, T.
author_facet Gaina, C.
Müller, R. D.
Brown, B.
Ishihara, T.
author_sort Gaina, C.
title Microcontinent formation around Australia
title_short Microcontinent formation around Australia
title_full Microcontinent formation around Australia
title_fullStr Microcontinent formation around Australia
title_full_unstemmed Microcontinent formation around Australia
title_sort microcontinent formation around australia
publisher Geological Society of America
publishDate 2003
url https://eprints.qut.edu.au/234263/
long_lat ENVELOPE(148.000,148.000,-47.500,-47.500)
ENVELOPE(67.000,67.000,-56.750,-56.750)
ENVELOPE(-150.083,-150.083,52.833,52.833)
geographic Ross Sea
Kerguelen
Indian
South Tasman Rise
Elan Bank
Gilbert Seamount
geographic_facet Ross Sea
Kerguelen
Indian
South Tasman Rise
Elan Bank
Gilbert Seamount
genre Antarc*
Antarctica
Ross Sea
genre_facet Antarc*
Antarctica
Ross Sea
op_source Evolution and Dynamics of the Australian Plate
op_relation doi:10.1130/0-8137-2372-8.405
Gaina, C., Müller, R. D., Brown, B., & Ishihara, T. (2003) Microcontinent formation around Australia. In Hillis, R. R. & Muller, R. D. (Eds.) Evolution and Dynamics of the Australian Plate. Geological Society of America, United States of America, pp. 405-416.
https://eprints.qut.edu.au/234263/
op_rights 2003 Geological Society of America, Inc.
This work is covered by copyright. Unless the document is being made available under a Creative Commons Licence, you must assume that re-use is limited to personal use and that permission from the copyright owner must be obtained for all other uses. If the document is available under a Creative Commons License (or other specified license) then refer to the Licence for details of permitted re-use. It is a condition of access that users recognise and abide by the legal requirements associated with these rights. If you believe that this work infringes copyright please provide details by email to qut.copyright@qut.edu.au
op_doi https://doi.org/10.1130/0-8137-2372-8.405
_version_ 1789959807270125568